Target Acquisition Reference Information . There are limits to the brightest and bluest stars that can be acquired with mirrors N1 and N2 because of the very high fluxes of these objects. Figure 7.3 on page 91 shows the limits for these two mirrors as set in the Constraints and Restrictions Document (CARD). ... Once you have predicted an acquisition count rate, you then determine the integration time per dwell point during the target acquisition: STEP-TIME. ... STEP-TIME Constraints . ...

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... User Portal . ... Science Users Information > Observing with ESO Telescopes > Phase 2 Preparation > Phase 2 Instrument Table . ... Phase 2 Instrument Table . ... Manuals and Tutorials . ... Calibration Plan . ... The P2PP Tool (version 3) . ... Phase 2 Users Workshops . ... If one instrument has special requirements, this is visualized in the relevant row of the table. A summary table of the main characteristics of all instruments is available here . Instrument . ... FAQ . ... User Manual . ...

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... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

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• Local HI: Constraints on the evolution of the HI content of the Universe
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... WMAP7 -- 7 year WMAP data ( Larson at al., ... SPT -- CMB power spectrum from SPT ( Keisler et al., ... CDM -- flat Universe with cosmological constant . ... N eff 3.046 . ... WCDM -- flat Universe with dark energy . ... CDM, WMAP7+BAO+H0 +CL . CDM, WMAP7+BAO+H0+SPT +CL . ... CDM+f (1), WMAP7+SPT+BAO+H0 +CL . CDM+f (1)+N eff , WMAP7+SPT+BAO+H0 +CL . ... CDM+N eff , WMAP7+BAO+H0 +CL . ... CDM+dn/dlnk, WMAP7+BAO+H0 +CL . ... WCDM, WMAP7+SPT+BAO+H0 +CL . ... WCDM, WMAP7+SPT+BAO+H0+SNSYS +CL . ...

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indicator: submit id: form attributes : method: post auto_fieldset: 1 elements: - type : Select name : tipo label : Tipo di utenza options: - ['', ''] - [' scuola ', ' scuola '] - ['privato', 'privato'] - ['associazione', 'associazione o gruppo'] constraints : - Required attributes : onblur: proper_display(this.value);goajax_prenotazioni('create') id: type - type : Text name : num_persone label : Numero di partecipanti ...

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leda -aladin v 0.6 (2002/04/18) This CGI process a coordinate-box request to LEDA , / leda Usage: #/ cgi-bin / leda-aladin.cgi ?ra=$1 de=$2 width =$3 height =$4 name =$5 type =$6 constraint =$7 $1: (ra) Right ascension J2000 in [deg] $2: (de) Declination J2000 in [deg] $3: ( width ) Width of the box [arcmin] $4: ( height ) Height of the box [arcmin] $5: ( name ) Designation of an object in If (type)="astrores", return an astrores document. ... Otherwise perform a search near position. ...

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• Access LEDA from Aladin

attach_mod schema - mssql $Id: attach_mssql_schema.sql,v 1.3 2003/01/29 11:43:58 acydburn Exp $ */ BEGIN TRANSACTION GO CREATE TABLE [phpbb_attachments_config] ( [config_name] [ varchar ] (100) NOT NULL , [config_value] [ varchar ] (100) NOT NULL ) ON [ PRIMARY ] GO CREATE TABLE [phpbb_forbidden_extensions] ( [ext_id] [ int ] IDENTITY (1, 1) NOT NULL , [extension] [char] (100) NOT NULL ) ON [ PRIMARY ] GO CREATE ...

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. First page Back Continue Last page Summary Graphics .

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• Slide 5
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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The black lines are contours of the ejected mass fraction 1 тИТ with values of, from left to right, 0.0, 0.1, and 0.9, respectively. The red lines mark contours of merger mass M 1 + M 2 = M ch (conservative case, solid line), M 1 + M 2 = M ch (non-conservative, dotted line), and M 1 + (t)M 2 (t)dt = M ch (non-conservative, dashed line). The vertical lines give the boundaries for M 1 = 0.9 and 1.0 M ? ...

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Next: Navigation Pre-Observation Products . ... SRT (Space Radio Telescope) Schedule (SRS) File . ... What: GOCG generates the Space Radio Telescope (SRT) schedule file, or SRS file, from current GSTS file. The SRS file has more precise time stamps than long-term schedules, and also designates which GTS will be used when. ... The SRS file also serves as the antenna pointing schedule file, as it describes the planned orientation of the spacecraft (and solar panels) as a function of time. ...

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• Description of the RadioAstron project, english version
• RadioAstron main page, english version
• Appendix A: Acronyms and Abbreviations

HOMOGENEOUS STUDIES OF TRANSITING PLANETS John Southworth Advanced Fellow Keele University, UK Mass versus radius planets on the left host stars on the right Homogeneous studies of transiting planets · Light curve fit: jktebop · Limb darkening: ­ five different laws · Contaminating light ­ constraints from highresolution imaging Light curve of WASP-2 (Southworth et al. ...

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... Matching the Surface of Best Focus . ... The plug-plates of SDSS project are responsible for locating the optical-fiber plugs spatially and for defining the plug tilt with respect to the surface of best focus. ... Approximately 670 holes are drilled in each plate. ... In the first attempts to match the curvature of the plug-plates to that of the best focal surface, the bending fixture was set upon 3 6.630mm metal supports that were affixed to a table top and spaced 120 apart. ...

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• Mirror baffle inspection
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... Green and blue curves - CYGAM telescope (squares - no constraints on the angle a , triangles - a <0.5 0 ); red curve - EGRET telescope. Effective area versus photon incidence angle to relative the longitudinal telescope axis (squares - no constraints on the angle a , triangles - a <0.5 0 , spectral index g= 2). ... Angular resolution for normal to the axis X incidence versus source power law spectrum index (squares- no constraints on the angle a , triangles- a <0,5 0 ). ... CYGAM (PDF, 450 Kb) . ...

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• Reports
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... It provides long range planning information to the scheduling team; it provides bright object, timing, and orientation information to the observation planning team; and it provides graphical description of the observations and their constraints. ... The GUI graphically displays the constraints that are computed by Spike and stored in the description files and in the database. ... BOAS processes all bright objects that have entered the database since the last time BOAS was run. ...

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... Семинар М.Э.Казаряна и С.К.Ландо "Характеристические классы и теория пересечений" возобновляет свою работу в четверг 4 сентября в 19.00 (обратите внимание на смену дня недели! аудитория уточняется). 11 сентября, четверг . ... As a result, we obtain a CohFT on the usual moduli space of curves whose correlators related to the original correlators of TCFT via Givental . 4 сентября, четверг . ...

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... Estimation of source coordinate time series from analysis of VLBI sessions. ... Conventions Cut-off elevation angle: 5є Terrestrial datum: NNR/NNT constraints to VTRF2008 stations without breaks (in total) For the sources : T L(2011) NNR Yes No s [ mas ] 2000 2000 Dip. ampl. [ mas /yr] 6.4 ±1.5 6.5 ±1.5 a (є) 263 ±11 263 ±11 d (є) -20 ±12 -23 ±12 Constraining each source to the ICRF2 position using very loose constraints (s=2as) is equivalent to apply loose NNR ...

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... D.1 Grammar . ... D.3 Comparison of tokenization in CSS2 and CSS1 . This appendix is normative. ... STRING ] S* ]? ']' ; pseudo : ':' [ IDENT | ... LENGTH S* | ... return CDC;} ~= { return INCLUDES;} |= { return DASHMATCH;} { string } { return STRING ;} { ident } { return IDENT ;} # {name} { return HASH;} @import { return IMPORT_SYM;} @page { return PAGE_SYM;} @media { return MEDIA_SYM;} @font-face { return FONT_FACE_SYM;} @charset { return CHARSET_SYM;} @ { ...

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... To address the problem of point-source photometry in restored images Lucy (1994) suggested a two-channel photometric restoration method in which the points are represented as functions in one channel and the background, constrained to be smooth by an additional entropy constraint, in the other. ... In the new CPLUCY implementation the stars can be at arbitrary x , y sub-pixel positions but the entropy constraint on the background, used by PLUCY, is retained. ...

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arxiv:1002.4415 Ограничения на космологический сигнал от аннигиляции темной материи по данным Fermi-LAT об изотропном гамма-фоне (Constraints on Cosmological Dark Matter Annihilation from the Fermi-LAT Isotropic Diffuse Gamma-Ray Measurement) . Authors: The Fermi-LAT collaboration . arxiv:1002.3205 Обнаружение задержанного ГэВного излучения от короткого гамма-всплеска 081024B по данным Ферми (Fermi detection of delayed GeV emission from the short GRB 081024B) . ... Authors: B. Scott Gaudi ...

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... 8, ``Celestial Mechanics'', 2002 Analytical constraints on comet nucleus rotation A. I. Neishtadt 1 , D. Scheeres 2 , V. V. Sidorenko 3 , A. A. Vasiliev 1 1 Space Research Institute, Moscow, Russia 2 University of Michigan, Ann Arbor, USA 3 Keldysh Institute of Applied Mathematics, Moscow, Russia Nucleus rotation essentially affects many processes studied in cometary phy­ sics. ... Peale S. J., Lissauer J. J. Rotation of Halley's comet. ... Wilhelm K. Rotation and precession of comet Halley. ...

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